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Diffraction-limited, 10-W, 5-ns, 100-kHz,

all-fiber laser at 1.55

μm

I. Pavlov,1,* E. Dülgergil,2E. Ilbey,1and F. Ö. Ilday1,3

1Department of Physics, Bilkent University, 06800 Ankara, Turkey

2Meteksan Savunma Inc., Ankara, Turkey

3Department of Electrical and Electronics Engineering, Bilkent University, 06800 Ankara, Turkey

*Corresponding author: [email protected]

Received December 30, 2013; revised March 25, 2014; accepted March 25, 2014; posted March 26, 2014 (Doc. ID 203874); published April 25, 2014

This Letter reports on an all-fiber-integrated master-oscillator, power amplifier system at 1.55μm producing 5-ns,

100-μJ pulses. These pulses are generated at a 100 kHz repetition rate, corresponding to 10 W of average power. The seed source is a low-power, current-modulated, single-frequency, distributed feedback semiconductor laser. System output is obtained from a standard single-mode fiber (Corning SMF-28). Consequently, the beam is truly diffraction

limited, which was independently proven byM2measurements. Further increase of peak power is limited by onset

of significant spectral broadening due to nonlinear effects, primarily four-wave mixing. Numerical simulations based on six-level rate equations with full position- and time-dependence were developed to model propagation of pulses through the amplifier chain. This capability allows minimization of the amplified spontaneous emission,

which can be directly measured using a fast acousto-optic modulator to gate the pulses. © 2014 Optical Society of

America

OCIS codes: (140.3510) Lasers, fiber; (060.2320) Fiber optics amplifiers and oscillators. http://dx.doi.org/10.1364/OL.39.002695

In the last decade, fiber laser development has focused on Yb-fiber lasers because of their excellent capacity for

high-power operation [1,2]. However, there are various

established and emerging applications that require the relative eye safety afforded by longer wavelength Er-fiber lasers. These applications include remote laser sensing

[3] and lidars [4], and require low-cost, mechanically

robust, high-energy pulsed laser sources with average power and repetition rates higher than reported so far, while maintaining excellent beam quality. Achievement of high peak powers is limited by the well-known difficul-ties arising from the strong nonlinear effects of confining beam propagation over several meters in the small core of a single-mode fiber (SMF). In addition to

four-wave-mixing, stimulated Raman scattering [5] and for narrow

line-width lasers, stimulated Brillouin scattering [5] are

the dominant effects, resulting in spectral broadening and in the extreme, destabilization of the laser operation or even damaging the components of the laser system.

The standard approach to reach high peak power is to reduce the nonlinear effects by using large-mode area

fi-bers [6–8]. Increasing the core diameter of the gain fiber

requires elaborate methods of higher-order mode sup-pression, which does not always succeed. For certain applications, however, the beam quality should be truly diffraction-limited, devoid of any higher-order modes. A guaranteed way to ensure pure single-mode operation is

to use standard SMF, such as SMF-28 [9].

In that case, the gain fiber length must be minimized to limit the nonlinear effects. Compared to Yb-doped fibers, Er-doped fibers have relatively low pump absorption lev-els, requiring long fiber lengths and resulting in enhanced nonlinear effects. This appears to be a primary reason behind the relatively poor peak-power performance of pulsed Er-fiber lasers compared to Yb-fiber lasers. Partial

relief comes from tandem pumping [10], which allows

shortening of the required gain fiber, reducing nonlinear effects indirectly. Codoping with Yb ions addresses the

issue of low pump absorption, also allowing for shorter gain lengths, but introduces a stronger spontaneous amplified emission (ASE) problem. A significant amount of ASE can be generated in the gain fiber even at a

rel-atively high repetition rate [11]. Recently, 200μJ, 200 ns

pulses with a low repetition rate (Hz range) were

dem-onstrated with 17 μm core diameter gain fiber by using

pulsed pump source, which allows suppression of ASE

content at such low repetition rate [12].

Accurate characterization of the ASE content in the time domain is crucial since several publications are

re-porting Er-fiber and Er–Yb-fiber systems at very low

rep-etition rates. We attribute these reports to inferral of the ASE content purely by analysis of the optical spectrum. This method inherently assumes that all ASE is broad-band, which is not necessarily true. In a multistage sys-tem, particularly with spectral filters between the stages, ASE can start to build up within a narrow spectral region matching that of the signal, becoming difficult to distin-guish from the signal. Direct time-domain characteriza-tion can help avoid this pitfall.

Here, we report on an all-fiber-integrated, master-oscillator power-amplifier (MOPA) system, where the

power amplifier is based on Er–Yb-codoped double-clad

(DC) fiber. The system produces more than 10 W of average

output power at 100 kHz repetition rate with∼5 ns pulse

duration and 100μJ of pulse energy. We proposed and used

a time-domain method to characterize the ASE content. We used narrowband filters to suppress ASE by the use of nar-row-band filters, time-gating using an acousto-optic modu-lator (AOM) as well as careful optimization of the number of amplifier stages and the repetition rate. This optimiza-tion is made possible by using an accurate numerical model, which, in addition to helping us reduce the ASE, al-lows effective use of gain depletion to achieve sub-5-ns pulses, starting from a seed source of 15 ns.

We have developed a numerical model to describe propagation and amplification of pulses in the multistage

May 1, 2014 / Vol. 39, No. 9 / OPTICS LETTERS 2695

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amplifier. The model is based on numerically solving time- and space-dependent rate equations for Er-doped

fiber (three-level system) and Er–Yb-codoped fiber

(six-level system) [13,14]. The simplified rate equations are

given below and Fig. 1 depicts the corresponding

energy diagram for the Er–Yb-codoped fiber:

_N6 Wp46N4− N6 − σ65N6− KtrN6N1− N3N4; (1) _N5 σ65N6− Ws54N5 Ws45N4− σ54N5 − KtrN5N1− N3N4; (2) _N3 Wp13N1− N3  KtrN6N1− N3N4 − σ32N3  KtrN5N1− N3N4; (3) _N2 σ32N3− Ws21N2 Ws12N1− σ21N2; (4) NEr N1 N2 N3; (5) NYb N4 N5 N6: (6)

Here, _Ni denotes the time derivative of Ni, which is

the number of ions in ith state, where i  1; …; 6. The

equation

Wp;sij hνPp;sp;sA

effδij 7

shows the probabilities for absorption and stimulated

emission transition from level i to level j, for pump

and signal, where Pp;s are the corresponding pump or

signal power, andhνp;s are the pump or signal photon

energy, respectively. Aeff is the effective core area, δij

are the stimulated emission/absorption transition

cross-sections from leveli to level j, and σijare the

prob-abilities of spontaneous transitions (radiative and

nonra-diative) from leveli to level j. Ktr is the energy transfer

coefficient between the Er and the Yb levels. These coupled equations are solved using finite differences method. This way, time- and space-resolved dynamics are considered, allowing us to account for processes such as dynamic gain saturation, which results in tempo-ral reshaping of the pulse and time-dependent ASE cre-ation. For the Er-only amplifier stages, the same model is used after simply eliminating the Yb levels and using the corresponding parameters.

Figure 2 shows simplified schematics of the

experi-mental setup. The number of amplifier stages, the relative gain factors achieved by them, the placement of the bandpass filters and the placement of the AOM have

all been optimized using the numerical simulations and through careful experimental characterization in an iter-ative procedure, culminating in the current design. As seed source, we use an electronically modulated distrib-uted feedback semiconductor laser (DFBL).

The current supplied to the DFBL is modulated elec-tronically to produce pulses of adjustable duration and as short as 15 ns. Since the DFBL is limited in the current it can handle, the maximum pulse energy is limited to about 1.5 nJ for this pulse duration. Thus, we operate it at 500 kHz, corresponding to 0.2 mW, to be able to sat-urate the first preamplifier that follows. The seed signal is

amplified in two preamplifiers, first in a 6.5μm mode field

diameter (MFD), 40-cm-long Er-fiber with absorption

level of80 dB∕m at 1530 nm to 9 mW (18 nJ) and then

in a 6.5 μm MFD, 120-cm-long Er-fiber with absorption

level of80 dB∕m at 1530 nm to 120 mW.

These two stages are pumped in core by a single pump diode (operating at 976 nm), the output of which is split to deliver 80 and 400 mW to the first and second pream-plifiers, respectively. ASE generation is kept in check with a bandpass filter of 100 GHz bandwidth. The pulses then traverse a fiber-coupled AOM, where the pulse train is gated with square pulses of temporal width of 100 ns to

reduce the repetition rate (to the range of 50–100 kHz).

In addition to lowering the repetition rate, the gating

operation (with a suppression coefficient of >50 dB)

blocks any ASE between the pulses.

Fig. 1. Schematic of energy levels for the Er–Yb codoped fiber.

Fig. 2. Schematic of the experiment setup. BF, bandpass filter; MM, multimode; SM, single-mode; MPC, multiple-port pump-signal combiner; WDM, wavelength division multiplexer; AOM, acousto-optic modulator; and DBFL, distributed feedback laser. 2696 OPTICS LETTERS / Vol. 39, No. 9 / May 1, 2014

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Due to the 50% insertion loss of the AOM, there are three additional amplifier stages. The first stage consists

of a 1.2 m Er-doped SMF (6.5μm MFD, core absorption of

80 dB∕m at 1530 nm), which also is core-pumped by a similar single-mode pump diode, amplifying the signal to 169 mW. The second stage is comprised of a 3 m DC

Er–Yb-codoped fiber with 10 μm core and 125 μm

clad-ding diameter (Coractive Inc.). The pump source is a

mul-timode diode at 976 nm coupled to a 105 μm fiber, the

output of which is delivered through a signal-pump com-biner (MPC) into the cladding region in the backward direction. A bandpass filter and an isolator follow, to reduce ASE and limit nonlinear spectral broadening, and to protect the amplifier from backward-propagating light from the final amplifier stage, respectively. The average signal power at this point reaches 1.2 W. The final power

amplifier stage is comprised of a 5.5-m-long DC Er

–Yb-codoped fiber with 12μm core and 130 μm cladding

diam-eter (Coractive Inc.), which also is backward pumped in the cladding by two high-power fiber-coupled multimode diodes at 976 nm through a MPC. Both second and third stages MPCs were commercially available (Lightcomm Technology) with 15 W of power handling for each pump port.

We did not apply any special precautions to ensure pump diodes from possible signal leakage to the pump ports. A fiber-pigtailed collimator, capable of handling high powers, is spliced to the signal port of MPC. The

final average output power reaches 10 W [Fig. 3(a)].

The fiber of the signal port of the combiner and that of the output collimator are both SMF-28, which is strictly

single-mode at 1.55μm and thus produces a near

diffrac-tion-limited, spatially Gaussian output beam of measured

M2 1.04 [Fig. 3(b)]. We stress that, although the final

amplifier fiber can in principle support multiple trans-verse modes (V 4.6), we observed no appreciable power loss coupling its output into the SMF-28 output pigtail. This shows that the optical power exiting the fiber am-plifier is predominantly confined within the fundamental LP01 mode.

For direct, time-domain characterization of the ASE content of the amplifier signal, a small part of the output signal can be channelled into a fiber-coupled AOM. If the

AOM is gated with a negative ∼100 ns square pulse,

synchronized to the pulse train, this operation drops only the pulse, revealing any ASE signal that has accumulated between the pulses. In this configuration, measurement of the ratio of the transmitted power with the pulse dropped to the power with AOM passing all the signal

gives the fraction of optical energy between the pulses (i.e., the ratio of ASE to the total signal). We consider this to be a more reliable method to assess ASE content that spectral measurements and the use of energy meters, which also can be misleading since the ASE signal is not

a strictly continuous wave [Fig. 4(a)] due to its

time-dependent buildup.

Theoretical calculations and experimental measure-ments demonstrate that operation of the laser system at repetition rates below 100 kHz results in steep increases

of ASE (Fig. 4). Even with long pulses and low peak

powers, which result in negligible spectral broadening, the presence of substantial amounts of ASE is not readily discernible from the optical spectrum, which remains nar-row due to the use of the bandpass filters. However, de-pending on the experimental conditions, the AOM-based measurement reveals that the amount of ASE varies be-tween 60% and 80% of the total output power at 50 kHz. Although it is impossible to time-resolve the ASE signal due to the small duty cycle and limited amplitude reso-lution (limited by 8-bit digitization) of an oscilloscope di-rectly, it is possible to qualitatively visualize the ASE build-up dynamics by strongly oversaturating a photo-detector, such that the gradual ASE buildup between

the pulses is resolved [Fig.4(a)]. We observe that ASE

starts to grow substantially about 10μs after each pulse.

This suggests that the repetition rate for our amplifier configuration should be around 100 kHz to limit ASE to between 2% and 4%. These experimental observations are consistent with earlier investigations of ASE creation

[11], where 17μm core gain fiber was used. Furthermore,

our numerical simulations are in good agreement with

the measurements [Fig. 4(b)].

Figure5presents the operational characteristics of the

system at 100 kHz. Amplified pulses of ∼5 ns duration

can routinely be obtained, corresponding to peak power as much as 20 kW at 10 W average power and 100 kHz. Due to the high peak power, we observed significant

spectral broadening after the last stage (Fig.5(a)).

How-ever, as confirmed by the direct ASE measurements, the ASE level is kept very low.

Due to dynamic gain saturation, the final pulse width depends sensitively on the frontal slope of the seed pulse, which can be used as a control parameter to tune the final pulse width. The pulse duration decreases significantly starting from 15 ns to less than 4 ns, but

0 20 40 60 80 100 0 1 2 3 4 Position (mm) Beam Diameter (mm) 0 5 10 15 20 25 30 0 2 4 6 8 10 12 Pump Power (W) Output Power (W) (a) (b) M2 = 1.04

Fig. 3. (a) Measured signal output power as a function of pump power for final stage amplifier. (b) Dependence of beam diameter at the 1/e-level on position, along with fittedM2value. Inset: far-field 3D beam profile.

40 60 80 100 120 140 1 10 100 Repetition Rate (kHz) ASE Ratio (%) −5 0 5 10 15 20 25 0 1 Time (µs) Intensity (a.u.) (a) (b)

Fig. 4. (a) Temporal profile of the amplified pulse train show-ing the ASE buildup at 50 kHz, where the vertical axis is not a linear function of power due to extreme saturation of the photo-detector to render the ASE signal visible. (b) Variation of the ASE ratio in the amplified signal as a function of repetition rate. Simulation and experimental results are represented by full and empty circles, respectively.

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we typically obtain 5 ns [Fig.4(b)]. The buildup of aver-age power in the final staver-age of amplification is accurately described by simulations, when compared to

experi-ments [Fig. 5(c)]. The evolution of the temporal shape

of the pulse within the amplifier illustrates the

well-known mechanism of pulse shortening [Fig.5(d)].

In conclusion, guided by a detailed, accurate numerical model and through careful experimental characteriza-tion, we have developed a truly single-mode laser source producing 10 W, 5 ns, 100 kHz pulses at the eye-safe

wavelength of 1.55 μm. The laser beam is always

con-fined in fiber or a fiberized component at all points, ren-dering the system immune to mechanical perturbations.

To the best of our knowledge, this is the highest pulse energy reported for strictly single-mode operation at this wavelength. Theoretical and experimental optimization suggest that operation at repetition rates below 100 kHz would require pulsed pumping to keep ASE levels below

10% when Er–Yb-codoped fiber is used. A detailed

theo-retical analysis of the ASE generation process and the ultimate limits to its minimization will be covered in a future publication. We expect this robust, high-power, diffraction-limited, yet compact and all-fiber laser system to find various applications, particularly in remote sens-ing and lidars.

This work was supported by the SANTEZ Project

No. 00255.STZ.2008-1 and by the SSM “Fiber Laser”

Project.

References

1. D. J. Richardson, J. Nilsson, and W. A. Clarkson, J. Opt. Soc. Am. B27, B63 (2010).

2. C. Jauregui, J. Limpert, and A. Tünnermann, Nat. Photonics 7, 861 (2013).

3. S. Gupta, D. Engin, K. Puffenberger, S. Litvinovich, F. Kimpel, and R. Utano, Proc. SPIE8876, 88760E (2013). 4. J. Lee, Y.-J. Kim, K. Lee, S. Lee, and S.-W. Kim, Nat.

Photon-ics4, 716 (2010).

5. G. Agrawal, Nonlinear Fiber Optics (Academic, 2006). 6. V. Philippov, C. Codemard, Y. Jeong, C. Alegria, J. K. Sahu,

J. Nilsson, and G. N. Pearson, Opt. Lett.29, 2590 (2004). 7. C. Codemard, C. Farrel, P. Dupriez, V. Philippov, J. K. Sahu,

and J. Nilson, C.R. Physique7, 170 (2006).

8. E. Petersen, W. Shi, A. Chavez-Pirson, and N. Peyghambarian, Appl. Opt.51, 531 (2012).

9. I. Pavlov, E. Ilbey, E. Dulgergil, A. Bayri, and F. O. Ilday, Opt. Express20, 9471 (2012).

10. E. Lim, S. Alam, and D. J. Richardson, Opt. Express20, 18803 (2012).

11. F. Di Teodoro, M. Savage-Leuchs, and M. Norsen, Electron. Lett.40, 1525 (2004).

12. P. Wan, J. Liu, L.-M. Yang, and F. Amzajerdian, Opt. Express 19, 18067 (2011).

13. B. Morasse, S. Agger, C. Hovington, S. Chatigny, E. Gagnon, J.-P. de Sandro, and C. Poulsen, Proc. SPIE6453, 645324 (2007).

14. M. Karasek, IEEE J. Quantum Electron.33, 1699 (1997). Fig. 5. (a) Measured optical spectra of the seed (dotted line)

and amplified pulses at full power (solid line). (b) Temporal profiles of the pulses: Seed pulse generated by the DFBL (dashed line), simulated (dotted line) and experimentally mea-sured (solid line) amplified pulses at full power. (c) Evolution of the average signal (solid line) and pump (dashed line) power along the final-stage fiber amplifier obtained from simulations. Measured signal (downward triangles) and pump (upward tri-angle) power show the good agreement between simulations and experiments. (d) Simulated evolution of the pulse as it propagates inside of the final-stage amplifier, showing the steepening of the leading edge due to gain depletion.

Şekil

Figure 2 shows simplified schematics of the experi- experi-mental setup. The number of amplifier stages, the relative gain factors achieved by them, the placement of the bandpass filters and the placement of the AOM have
Fig. 3. (a) Measured signal output power as a function of pump power for final stage amplifier
Fig. 5. (a) Measured optical spectra of the seed (dotted line) and amplified pulses at full power (solid line)

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